Astronomy:Ymir (moon)

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Short description: Moon of Saturn
Ymir
Ymir-discovery-eso0036a (cropped).jpg
Discovery image of Ymir taken by the La Silla Observatory in August 2000
Discovery[1]
Discovered byBrett J. Gladman
Discovery siteObservatoire de la Cote d'Azur
Discovery date2000
Designations
Designation
Saturn XIX
Pronunciation/ˈmɪər/,[2] /ˈɪmɪər/[3]
Named afterYmir
S/2000 S 1
AdjectivesYmirian /ɪˈmɪəriən/[4][5]
Orbital characteristics[6]
23,040,000 km
Eccentricity0.3349
Orbital period3.6 yr (1315.14 d)
Mean anomaly244.521°
Inclination173.125°
Longitude of ascending node194.086°
22.668°
Satellite ofSaturn
GroupNorse group
Physical characteristics
Mean diameter19+50%
−30%
 km
[7]
Rotation period11.92220±0.00002 h[7]
11 h 55 m 20 s[8]
Albedo0.06[9]
Spectral type
D/P[8]


Ymir /ˈmɪər/, or Saturn XIX, is the second-largest retrograde irregular moon of Saturn. It was discovered by Brett J. Gladman, et al. in 2000, and given the temporary designation S/2000 S 1. It was named in August 2003 after Ymir, who in Norse mythology is the ancestor of all the Jotuns or frost giants.[10]

It takes 3.6 Earth years to complete an orbit around Saturn. Of the moons that take more than 3 Earth years to orbit Saturn, Ymir is the largest, at about 18 kilometres (11 miles) in diameter;[11] Ymir is also the second largest member of the Norse group, after Phoebe.[8]

Spectral measurements from Cassini–Huygens show that Ymir is reddish in color, unlike Phoebe's gray color, suggesting a separate origin for this moon.[8] It shows a similar light curve as Siarnaq and has a triangular shape, rotating in a retrograde direction about once every 11.9 hours.[8]

Ymir imaged by the CFHT on 23 September 2000

References

  1. Brian G. Marsden (2000-10-25). "IAUC 7512". IAU. http://www.cbat.eps.harvard.edu/iauc/07500/07512.html. 
  2. "Ymir". Merriam-Webster Dictionary. https://www.merriam-webster.com/dictionary/Ymir. 
  3. Merriam-Webster's Encyclopedia of Literature. 1995. 
  4. Budd (1898). "Norse Mythology". St. Mary's Hall lectures: and other papers. p. 84.  Because the -r is an inflectional ending, and the oblique stem is Ymi (as in Modern Norse Yme), one might expect the English adjective to be ?Ymian, but that is perhaps too short a word to be easily intelligible.
  5. James Hall III (2015). Moons of the Solar System. p. 107. 
  6. Jacobson, R.A. (2007) SAT270, SAT271 (2007-06-28). "Planetary Satellite Mean Orbital Parameters". JPL/NASA. http://ssd.jpl.nasa.gov/?sat_elem#saturn. 
  7. 7.0 7.1 Denk, T.; Mottola, S. (2019). "Cassini Observations of Saturn's Irregular Moons". 50th Lunar and Planetary Science Conference. Lunar and Planetary Institute. https://www.hou.usra.edu/meetings/lpsc2019/pdf/2654.pdf. 
  8. 8.0 8.1 8.2 8.3 8.4 T. Denk, S. Mottola, F. Tosi, W.F. Bottke, D.P. Hamilton (2018). The Irregular Satellites of Saturn. Space Science Series, The University of Arizona Press, Tucson, AZ. Chapter 20. 409–434. doi:10.2458/azu_uapress_9780816537075-ch020. ISBN 9780816537075. Bibcode2018eims.book..409D. https://tilmanndenk.de/wp-content/uploads/DenkEtAl2018_IrregularMoons.pdf. 
  9. Nicholson, P. D. 2001
  10. Daniel W. E. Green (2003-08-08). "IAUC 8177: Sats OF (22); Sats OF JUPITER, SATURN, URANUS". IAU. http://www.cbat.eps.harvard.edu/iauc/08100/08177.html. 
  11. Cite error: Invalid <ref> tag; no text was provided for refs named sheppard

External links